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密近双星自转的测量和研究(V) 轨道圆化
谭徽松; 潘开科
1997
Source Publication天体物理学报
ISSN0253-2379
Volume017Issue:004Pages:386
Abstract作为密近双星自转测量和研究的系列文章之一,本文从轨道圆化的角度讨论了Zahn的动力学潮汐机制粘滞理论、Tassoul的纯流体动力学理论与实测数据的简便程度,对前前文中的29个不相接双星系统,均分别计算了出以上理论所预测匠轨道沦时标,分析比较了各系统的理论圆化时标与它的年龄及轨道圆化和蔼间的关系,结果表明:动力学潮汐、粘滞理论的计算结果出比纯流体动力学机制的预期更符合实测数据,但与文(IV)的结果相
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/42711
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
谭徽松,潘开科. 密近双星自转的测量和研究(V) 轨道圆化[J]. 天体物理学报,1997,017(004):386.
APA 谭徽松,&潘开科.(1997).密近双星自转的测量和研究(V) 轨道圆化.天体物理学报,017(004),386.
MLA 谭徽松,et al."密近双星自转的测量和研究(V) 轨道圆化".天体物理学报 017.004(1997):386.
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